Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-14T05:42:48.375Z Has data issue: false hasContentIssue false

The source of heavy organics and aerosols in Titan's atmosphere

Published online by Cambridge University Press:  01 February 2008

J. H. Waite Jr.
Affiliation:
Southwest Research Institute, San Antonio, TX. 78228, email: hwaite@swri.edu
D. T. Young
Affiliation:
Southwest Research Institute, San Antonio, TX. 78228, email: hwaite@swri.edu
A. J. Coates
Affiliation:
Mullard Space Science Laboratory, University College London
F. J. Crary
Affiliation:
Southwest Research Institute, San Antonio, TX. 78228, email: hwaite@swri.edu
B. A. Magee
Affiliation:
Southwest Research Institute, San Antonio, TX. 78228, email: hwaite@swri.edu
K. E. Mandt
Affiliation:
Southwest Research Institute, San Antonio, TX. 78228, email: hwaite@swri.edu
J. H. Westlake
Affiliation:
Southwest Research Institute, San Antonio, TX. 78228, email: hwaite@swri.edu Unversity of Texas at San Antonio, San Antonio, TX. 78249
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Ion-neutral chemistry in Titan's upper atmosphere (~ 1000 km altitude) is an unexpectedly prodigious source of hydrocarbon-nitrile compounds. We report observations from the Cassini Ion Neutral Mass Spectrometer (INMS; Waite et al. 2004) and Cassini Plasma Spectrometer (CAPS; Young et al. 2004) that allow us to follow the formation of the organic material from the initial ionization and dissociation of nitrogen and methane driven by several free energy sources (extreme ultraviolet radiation and energetic ions and electrons) to the formation of negative ions with masses exceeding 10,000 amu.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Coates, A. J., Crary, F. J., Lewis, G. R., Young, D. T., Waite, J. H. Jr., & Sittler, E. C. Jr. 2007, Geophys. Res. Lett., 34, L22103, doi:10.1029/2007GL030978.Google Scholar
Conrath, B. J. 1985, ESA-SP-241, ESTEC.Google Scholar
Crary, , et al. , in preparationGoogle Scholar
Cui, , et al. , in preparationGoogle Scholar
Fox, J. & Yelle, R. 1997, Geophys. Res. Lett., 24 (17), 2179CrossRefGoogle Scholar
Kasprzak, , et al. , in preparationGoogle Scholar
Kuiper, G. P. 1944, ApJ, 100, 378CrossRefGoogle Scholar
Liang, M. C., Heays, A. N., Lewis, B. R., Gibson, S. T., & Yung, Y. L. 2007, ApJ (Letters), 664, L115CrossRefGoogle Scholar
Lopez, R. M. C., Elachi, C., Paganelli, F., Mitchell, K., Stofan, E., Wood, C., Kirk, R., Lorenz, R., Lunine, J., Wall, S. and Cassini RADAR Team, 2005, Flows on the surface of Titan as revealed by the Cassini RADAR, Bull. Am. Astron. Soc., 37, 739Google Scholar
Lorenz, R. D., et al. 2008, Geophys. Res. Lett., 35, 2206CrossRefGoogle Scholar
Magee, , et al. , in preparationGoogle Scholar
Sagan, C., Thompson, W. R., & Khare, B. N. 1992, Accounts Chem. Res., 25, 286CrossRefGoogle Scholar
Tomasko, M. G., Doose, L., Engel, S., Dafoe, L. E., West, R., Lemmon, M., Karkoschka, E., & See, C. 2007, Planetary and Space Science, doi:10.1016/j.pss.2007.10.012CrossRefGoogle Scholar
Vinatier, S., Bézard, B., Fouchet, T., Teanby, N. A., de Kok, R., Irwin, P. G. J., Conrath, B. J., Nixon, C. A., Romani, P. N., Flasar, F. M., & Coustenis, A. 2007, Icarus, 188, 120CrossRefGoogle Scholar
Vuitton, V., Yelle, R. V., & McEwan, M. J. 2007, Icarus, 191, 722CrossRefGoogle Scholar
Waite, J. H. Jr., Lewis, W. S., Kasprzak, W. T., et al. 2004, Space Sci. Rev., 114, 113CrossRefGoogle Scholar
Waite, J. H. Jr., Young, D. T., Cravens, T. E., Coates, A. J., Crary, F. J., Magee, B., & Westlake, J. 2007, Science, 316, 870CrossRefGoogle Scholar
Waite, J. H. Jr., et al. , in preparation (isotope paper)Google Scholar
Wilson, E. H. & Atreya, S. K. 2004, J. Geophys. Res., 109, E06002Google Scholar
Young, D. T., Berthelier, J. J., Blanc, M. et al. 2004, Space Sci. Rev., 114, 1CrossRefGoogle Scholar